A dynamical approach to the study of the bright young associations in the Large Magellanic Cloud

Details A dynamical approach to the study of the bright young associations in the Large Magellanic Cloud A dynamical approach to the study of the bright young associations in the Large Magellanic Cloud

Jan 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988pasp..100...37p&link_type=abstract

Astronomical Society of the Pacific, Publications (ISSN 0004-6280), vol. 100, Jan. 1988, p. 37-53. Research supported by Brigham

Astronomy and Astrophysics

Astronomy

2

Globular Clusters, Magellanic Clouds, Star Formation, Stellar Luminosity, Stellar Models, Mass To Light Ratios, Stellar Evolution, Stellar Spectrophotometry

Scientific paper

A model is presented and discussed in order to investigate how the dynamical properties of a young globular cluster depend on the details of the process of formation. Several parameters are constrained by applying the model to some massive associations. Values of a number of observables are obtained. The approach provided in the paper shows how, qualitatively, the evolution of a newly formed object, after the gas cloud expulsion, is affected by the features of the physical environment wherein the formation process takes place.

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